Kepler's immense photometric precision to date was maintained through
satellite stability and precise pointing. In this white paper, we argue that
image modeling--fitting the Kepler-downlinked raw pixel data--can vastly
improve the precision of Kepler in pointing-degraded two-wheel mode. We argue
that a non-trivial modeling effort may permit continuance of photometry at
10-ppm-level precision. We demonstrate some baby steps towards precise models
in both data-driven (flexible) and physics-driven (interpretably parameterized)
modes. We demonstrate that the expected drift or jitter in positions in the
two-weel era will help with constraining calibration parameters. In particular,
we show that we can infer the device flat-field at higher than pixel
resolution; that is, we can infer pixel-to-pixel variations in intra-pixel
sensitivity. These results are relevant to almost any scientific goal for the
repurposed mission; image modeling ought to be a part of any two-wheel
repurpose for the satellite. We make other recommendations for Kepler
operations, but fundamentally advocate that the project stick with its core
mission of finding and characterizing Earth analogs. abridged
Beschreibung
[1309.0653] Maximizing Kepler science return per telemetered pixel: Detailed models of the focal plane in the two-wheel era
cite arxiv:1309.0653Comment: A white paper submitted in response to the "Kepler Project Office Call for White Papers: Soliciting Community Input for Alternate Science Investigations for the Kepler Spacecraft"; 24 pages in length (that is, 14 pages over the white-paper page limit)
%0 Generic
%1 hogg2013maximizing
%A Hogg, David W.
%A Angus, Ruth
%A Barclay, Tom
%A Dawson, Rebekah
%A Fergus, Rob
%A Foreman-Mackey, Dan
%A Harmeling, Stefan
%A Hirsch, Michael
%A Lang, Dustin
%A Montet, Benjamin T.
%A Schiminovich, David
%A Schölkopf, Bernhard
%D 2013
%K 2013 Kepler a:Hogg planets proposal
%T Maximizing Kepler science return per telemetered pixel: Detailed models
of the focal plane in the two-wheel era
%U http://arxiv.org/abs/1309.0653
%X Kepler's immense photometric precision to date was maintained through
satellite stability and precise pointing. In this white paper, we argue that
image modeling--fitting the Kepler-downlinked raw pixel data--can vastly
improve the precision of Kepler in pointing-degraded two-wheel mode. We argue
that a non-trivial modeling effort may permit continuance of photometry at
10-ppm-level precision. We demonstrate some baby steps towards precise models
in both data-driven (flexible) and physics-driven (interpretably parameterized)
modes. We demonstrate that the expected drift or jitter in positions in the
two-weel era will help with constraining calibration parameters. In particular,
we show that we can infer the device flat-field at higher than pixel
resolution; that is, we can infer pixel-to-pixel variations in intra-pixel
sensitivity. These results are relevant to almost any scientific goal for the
repurposed mission; image modeling ought to be a part of any two-wheel
repurpose for the satellite. We make other recommendations for Kepler
operations, but fundamentally advocate that the project stick with its core
mission of finding and characterizing Earth analogs. abridged
@misc{hogg2013maximizing,
abstract = {Kepler's immense photometric precision to date was maintained through
satellite stability and precise pointing. In this white paper, we argue that
image modeling--fitting the Kepler-downlinked raw pixel data--can vastly
improve the precision of Kepler in pointing-degraded two-wheel mode. We argue
that a non-trivial modeling effort may permit continuance of photometry at
10-ppm-level precision. We demonstrate some baby steps towards precise models
in both data-driven (flexible) and physics-driven (interpretably parameterized)
modes. We demonstrate that the expected drift or jitter in positions in the
two-weel era will help with constraining calibration parameters. In particular,
we show that we can infer the device flat-field at higher than pixel
resolution; that is, we can infer pixel-to-pixel variations in intra-pixel
sensitivity. These results are relevant to almost any scientific goal for the
repurposed mission; image modeling ought to be a part of any two-wheel
repurpose for the satellite. We make other recommendations for Kepler
operations, but fundamentally advocate that the project stick with its core
mission of finding and characterizing Earth analogs. [abridged]},
added-at = {2013-09-04T14:23:48.000+0200},
author = {Hogg, David W. and Angus, Ruth and Barclay, Tom and Dawson, Rebekah and Fergus, Rob and Foreman-Mackey, Dan and Harmeling, Stefan and Hirsch, Michael and Lang, Dustin and Montet, Benjamin T. and Schiminovich, David and Schölkopf, Bernhard},
biburl = {https://www.bibsonomy.org/bibtex/26ffc65ab3ef432c716bb657a1b758876/danielcarrera},
description = {[1309.0653] Maximizing Kepler science return per telemetered pixel: Detailed models of the focal plane in the two-wheel era},
interhash = {7bc8c0075732d267eddab9c336af995f},
intrahash = {6ffc65ab3ef432c716bb657a1b758876},
keywords = {2013 Kepler a:Hogg planets proposal},
note = {cite arxiv:1309.0653Comment: A white paper submitted in response to the "Kepler Project Office Call for White Papers: Soliciting Community Input for Alternate Science Investigations for the Kepler Spacecraft"; 24 pages in length (that is, 14 pages over the white-paper page limit)},
timestamp = {2013-09-06T13:26:50.000+0200},
title = {Maximizing Kepler science return per telemetered pixel: Detailed models
of the focal plane in the two-wheel era},
url = {http://arxiv.org/abs/1309.0653},
year = 2013
}